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  • Letter

Raising galaxy rotation curves via dressing

J. François*

L. Ravera†

  • *Contact author: jordan.francois@uni-graz.at
  • †Contact author: lucrezia.ravera@polito.it

Phys. Rev. D 112, L081501 – Published 6 October, 2025

DOI: https://doi.org/10.1103/m9xl-9vvk

Abstract

We present a manifestly diffeomorphism-invariant simple model of galaxy dynamics obtained by applying the dressing field method (DFM) to a general relativistic system comprising the metric and four scalar fields, phenomenologically representing the four-velocity of a cosmological fluid or dust field. The DFM, a systematic tool for extracting the gauge-invariant content in general relativistic theories, provides a physical coordinatization that yields corrective terms to the rotational velocity profile. These corrections produce galaxy rotation curves that combine Keplerian and constant velocity terms, effectively emulating a dark matter contribution. We compare DFM-derived rotation curves to observed data for spiral galaxies, from the Spitzer Photometry and Accurate Rotation Curves database, showing that the DFM allows one to fit them well.

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